Fullerenes in Space
John P Maier1, Ewen K Campbell1
1Department of Chemistry, University of Basel, Klingelbergstrasse 80, Basel, 4056, Switzerland.
Angewandte Chemie (International Ed. in English)
|January 11, 2017
Summary
The detection of buckminsterfullerene ions (C60+) in interstellar space has finally explained the long-standing mystery of diffuse interstellar bands. Sophisticated laboratory experiments confirmed C60+ as the source of these enigmatic spectral features.
Area of Science:
- Astrochemistry
- Spectroscopy
- Materials Science
Background:
- The diffuse interstellar bands (DIBs) are absorption features in starlight, observed for a century, with their molecular carriers remaining unidentified.
- Buckminsterfullerene (C60) was proposed in 1985 and synthesized in 1990, with its potential role in space considered early on.
Purpose of the Study:
- To identify the molecular carriers responsible for the diffuse interstellar bands.
- To confirm the presence and spectral signature of the buckminsterfullerene ion (C60+) in interstellar space.
Main Methods:
- Laboratory measurement of C60+ absorption spectra under cryogenic conditions (5 K neon matrix and conditions simulating diffuse clouds).
- Comparison of laboratory spectra with astronomical observations of diffuse interstellar bands.
- Analysis of astronomical data for absorption features in predicted wavelength ranges.
Main Results:
- Early laboratory spectra of C60+ (1993) predicted its absorption bands.
- Two diffuse interstellar bands were discovered in the predicted spectral region in 1994.
- Sophisticated laboratory experiments in 2015 confirmed that C60+ is responsible for these specific diffuse interstellar bands.
Conclusions:
- The buckminsterfullerene ion (C60+) has been definitively identified as the carrier of two prominent diffuse interstellar bands.
- This discovery provides the first molecular identification for these century-old astronomical observations.
- The study highlights the importance of laboratory astrophysics in solving interstellar mysteries.
More Related Videos
Related Concept Videos
Schwarzschild Radius and Event Horizon
2.9K
No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
2.9K
Rocket Propulsion In Empty Space - II
3.6K
The motion of a rocket is governed by the conservation of momentum principle. A rocket's momentum changes by the same amount (with the opposite sign) as the ejected gases. As time goes by, the rocket's mass (which includes the mass of the remaining fuel) continuously decreases, and its velocity increases. Therefore, the principle of conservation of momentum is used to explain the dynamics of a rocket's motion. The ideal rocket equation gives the change in velocity that a rocket...
3.6K
Rocket Propulsion in Empty Space - I
3.9K
The driving force for the motion of any vehicle is friction, but in the case of rocket propulsion in space, the friction force is not present. The motion of a rocket changes its velocity (and hence its momentum) by ejecting burned fuel gases, thus causing it to accelerate in the direction opposite to the velocity of the ejected fuel. In this situation, the mass and velocity of the rocket constantly change along with the total mass of ejected gases. Due to conservation of momentum, the...
3.9K
Nuclear Transmutation
20.9K
Nuclear transmutation is the conversion of one nuclide into another. It can occur by the radioactive decay of a nucleus, or the reaction of a nucleus with another particle. The first manmade nucleus was produced in Ernest Rutherford’s laboratory in 1919 by a transmutation reaction, the bombardment of one type of nuclei with other nuclei or with neutrons. Rutherford bombarded nitrogen-14 atoms with high-speed α particles from a natural radioactive isotope of radium and observed...
20.9K
Nuclear Fusion
34.1K
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
34.1K
π Molecular Orbitals of 1,3-Butadiene
12.4K
Conjugated dienes have lower heats of hydrogenation than cumulated and isolated dienes, making them more stable. The enhanced stabilization of conjugated systems can be understood from their π molecular orbitals.
The simplest conjugated diene is 1,3-butadiene: a four-carbon system where each carbon is sp2-hybridized and has an unhybridized p orbital that contains an unpaired electron. According to molecular orbital theory, atomic orbitals combine to form molecular orbitals such that the number...
The simplest conjugated diene is 1,3-butadiene: a four-carbon system where each carbon is sp2-hybridized and has an unhybridized p orbital that contains an unpaired electron. According to molecular orbital theory, atomic orbitals combine to form molecular orbitals such that the number...
12.4K


